The Search for Life in the Solar System - PowerPoint PPT Presentation

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The Search for Life in the Solar System

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Terrestrial Planets, Jovian Planets, other bodies. Environment for Life? ... Different densities of the planets are explained by condensation temperatures ... – PowerPoint PPT presentation

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Title: The Search for Life in the Solar System


1
The Search for Life in the Solar System
  • HNRS 228 w/Geller
  • Reviewing Chapter 6

2
Whats Up
  • Review Requirements for Life
  • Elements, Energy, Water, etc.
  • Searching for Life in Our Solar System
  • Remote Sensing, Robotics, Human Exploration, etc.
  • Biological Tour of the Solar System
  • Terrestrial Planets, Jovian Planets, other bodies

3
Environment for Life?
  • Source of elements to build cells
  • Source of energy
  • Medium for transporting molecules

4
H2O and CO2 Phase Diagrams (IMPORTANT
environmental consideration)
5
Exploring the Solar System
  • Observations from Earth
  • ground or orbit based
  • Robotic spacecraft
  • flybys, orbitals
  • landers
  • Human exploration

6
Planet Generalization
  • Terrestrial planets are closer to sun
  • Mercury
  • Venus
  • Earth
  • Mars
  • Jovian planets furthest from sun
  • Jupiter
  • Saturn
  • Uranus
  • Neptune

7
Planetary Summary
8
Some Conclusions
  • Planets formed at same time as sun
  • Planetary and satellite/ring systems are similar
    to remnants of dusty disks such as that seen
    about stars being born (e.g. T Tauri stars)
  • Planet composition dependent upon where it formed
    in solar system

9
Nebular Condensation Model
  • Most remnant heat from collapse retained near
    center
  • After sun ignites, remaining dust reaches an
    equilibrium temperature
  • Different densities of the planets are explained
    by condensation temperatures
  • Nebular dust temperature increases to center of
    nebula

10
Nebular Condensation Physics
  • Energy absorbed per unit area from sun energy
    emitted as thermal radiator
  • Solar Flux Lum (Sun) / 4 x distance2
  • Flux emitted constant x T4 Stefan-Boltzmann
  • Concluding from above yields
  • T constant / distance0.5

11
Nebular Condensation Chemistry
12
Nebular Condensation Summary
  • Solid Particles collide, stick together, sink
    toward center
  • Terrestrials -gt rocky
  • Jovians -gt rocky core ices light gases
  • Coolest, most massive collect H and He
  • More collisions -gt heating and differentiating of
    interior
  • Remnants flushed by solar wind
  • Evolution of atmospheres

13
Biological Tour of the Solar System
  • Consider problems posed for life on each of the
    following
  • Moon
  • Mercury
  • Venus
  • (Mars will be discussed in Chapter 7)
  • Jovian Planets
  • Other Moons
  • Asteroid, comets and other debris

14
Some References
  • The Search for Life (especially in the solar
    system)
  • http//www.scibridge.sdsu.edu/coursemats/introsci/
    Solarsys/lecture.html
  • http//www.resa.net/nasa/ocean_hydrothermal.htm
  • http//www.nationalacademies.org/ssb/lifeoriginsme
    nu.htm
  • http//www.phy.syr.edu/courses/modules/SETI/where.
    html
  • Books
  • Life on Other Worlds (Dick)
  • Cradle of Life (Schopf)
  • Life Everywhere (Darling)
  • Life on Other Worlds and How to Find It (Clark)
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